University of Crete HEP Seminars


FP7

Higher form symmetries and superfluids

Speaker: Diego Hofman
Institution: University of Amsterdam
Time: Monday 23 September 2019, 14:15
Venue: 2nd floor seminar room
Abstract: I will describe superfluid hydrodynamics as the hydrodynamic theory of a system with an emergent anomalous higher-form symmetry. The higher-form charge counts the winding planes of the superfluid -- its constitutive relation replaces the Josephson relation of conventional superfluid hydrodynamics. This formulation puts all hydrodynamic equations on equal footing. The anomalous Ward identity can be used as an alternative starting point to prove the existence of a Goldstone boson, without reference to spontaneous symmetry breaking. This provides an alternative characterization of Landau phase transitions in terms of higher-form symmetries and their anomalies instead of how the symmetries are realized. This treatment is more general and, in particular, includes the case of BKT transitions.

Dark matter search and gravitational wave detection using atom interferometry

Speaker: Wolf von Klitzing
Institution: IESL-FORTH Crete
Time: Thursday 26 September 2019, 14:15
Venue: 2nd floor seminar room
Abstract: In a recent White Paper (arXiv:1908.00802) we proposed a concept for a space experiment using cold atoms to search for ultra-light dark matter, and to detect gravitational waves in the frequency range between the most sensitive ranges of LISA and the terrestrial LIGO/Virgo/KAGRA/INDIGO experiments. This interdisciplinary experiment, called Atomic Experiment for Dark Matter and Gravity Exploration (AEDGE), will also complement other planned searches for dark matter, and exploit synergies with other gravitational wave detectors. We give examples of the extended range of sensitivity to ultra- light dark matter offered by AEDGE, and how its gravitational-wave measurements could explore the assembly of super-massive black holes, first-order phase transitions in the early universe and cosmic strings. AEDGE will be based upon technologies now being developed for terrestrial experiments using cold atoms (also on Crete), and will benefit from the space experience obtained with, e.g., LISA and cold atom experiments in microgravity.

The Geometric Trinity of Gravity: the TEGR case

Speaker: Konstantinos Dialektopoulos
Institution: Center for Gravitation and Cosmology, Yangzhou University
Time: Friday 27 September 2019, 16:15
Venue: 2nd floor seminar room
Abstract: It is well established by now that General Relativity and the LCDM model are very successful in describing the gravitational interactions at all scales. However, the theory is plagued with some shortcomings, enabling scientists to pursue an alternative formulation of gravity. In this talk, I am going to review the three different formulations of gravity; one based on the curvature of spacetime (General Relativity), one based on its torsion (Teleparallel Equivalent of General Relativity, TEGR) and one based on its non-metricity (Symmetric Teleparallel of General Relativity, STEGR). I will try to focus on the TEGR, explaining some of its key features.

Fine Tuning Problems from Cosmological Coleman-Weinberg Potentials

Speaker: Richard Woodard and S.P. Miao
Institution: UF (USA) and NCKU (Taiwan)
Time: Monday 21 October 2019, 14:15
Venue: 2nd floor seminar room
Abstract: Cosmological Coleman-Weinberg potentials are quantum corrections to the effective potential of the inflaton which result from coupling it to ordinary matter in order make re-heating efficient. These corrections are problematic for inflation because they are not Planck-suppressed and tend to make the potential too steep. Therefore they must be subtracted off by additions to the classical action. Unfortunately, they cannot be completely subtracted off. Although they go over to the Coleman-Weinberg form in the flat space limit, their actual form on de Sitter background is the 4th power of the Hubble parameter times a complicated function of the coupling constant times the ratio of the inflaton to the Hubble parameter. On a general inflationary background they are not even local functions of the geometry, whereas the allowable subtractions consist of algebraic functions of the inflaton and the Ricci scalar. We discuss the disturbing results from the best possible local subtraction schemes. This talk is based on arXiv:1506.07306, 1806.02533, 1908.03814 and 1908.05558.

Comments on the black hole S-matrix

Speaker: Panagiotis Betzios
Institution: UOC
Time: Tuesday 5 November 2019, 14:15
Venue: 2nd floor seminar room
Abstract: I will review the shockwave construction of 't Hooft by which gravitational backreaction can lead to a unitary S-matrix for particles scattering on an eternal black hole background. In order to obtain a background with a single exterior, an antipodal (CPT) identification was recently proposed that could in principle give a resolution to the information paradox for single sided asymptotically flat black holes. An emphasis will be given in the various assumptions and caveats of this construction. I will then describe an explicit dynamical quantum mechanical system that results in the same S-matrix. If time permits I will conclude with some efforts towards understanding the experience of an infalling observer in this setup.

The Skyrmion Paradox

Speaker: Christos Panagopoulos
Institution: NTU Singapore
Time: Tuesday 12 November 2019, 14:15
Venue: 2nd floor seminar room
Abstract: Magnetic skyrmions (or vortices) are spatially inhomogeneous spin textures localized in nanoscale cylindrical regions. Topological protection and small size make skyrmions especially attractive for the study of spin topology and technologies wherein information is carried by the electron spin further to, or instead of the electron charge. Despite achievements in the synthesis of materials where axisymmetric magnetic skyrmions can be stabilized and characterized, there is disproportionate progress in elucidating the basic properties. The talk will attempt to bridge this gap and deliver an intelligible guide on the physical principles governing these magnetic whirls.

Bootstrapping three dimensional cubic theories

Speaker: Stefanos Kousvos
Institution: UOC
Time: Thursday 14 November 2019, 14:15
Venue: 2nd floor seminar room
Abstract: After a concise introduction to the conformal bootstrap in general dimensions, I will discuss recent results regarding theories with cubic global symmetry in three spatial dimensions. Under certain assumptions, we find an isolated region in parameter space, which given prior intuition with the numerical conformal bootstrap, hints towards the existence of a CFT in this region of parameter space. We study the consistency of this CFT using multiple correlator systems. We find critical exponents for the conjectured CFT which are in discrepancy with the epsilon expansion (but in agreement with experiments for structural phase transitions). The disagreement of critical exponents for structural phase transitions calculated in the epsilon expansion with those measured in experiments is something that was noticed since the 70s. Given time I will briefly mention a resolution to this apparent discrepancy proposed at that time.

Violation of the horizon effect after a quantum quench in the sine-Gordon model

Speaker: Spyros Sotiriadis
Institution: University of Ljubljana
Time: Tuesday 4 February 2020, 14:15
Venue: 2nd floor seminar room
Abstract: The study of non-equilibrium dynamics in quantum field theories is of central importance for a wide range of physics areas, from high-energy and cosmology to condensed matter and atomic physics. One of the most characteristic features of quantum dynamics in relativistic field theories (and more generally systems characterised by a maximum speed of information propagation) is the "light-cone spreading" of correlations, also known as "horizon effect": starting from an initially short-range correlated state, measurements of two observers at distant points are expected to remain independent until their past light-cones start overlapping. Surprisingly, we find that in the presence of topological excitations, correlations can develop outside of the horizon, even between infinitely distant points. We demonstrate this effect in the sine-Gordon model, showing that it can be attributed to the non-local nature of its topological excitations and interpret it as dynamical emergence of entanglement at large distances. Our findings are derived in two independent ways: (i) a novel numerical technique for the simulation of quantum many-body dynamics in continuous models, and (ii) an exact analytical method based on the duality between sine-Gordon and massive Thirring model. References: Phys. Rev. Lett. 121, 110402 (2018) arXiv:1802.08696 arXiv:1906.02750

The Origin of the Six-Particle Amplitude at Finite Coupling

Speaker: Georgios Papathanasiou
Institution: DESY
Time: Thursday 6 February 2020, 14:15
Venue: 2nd floor seminar room
Abstract: Scattering amplitudes form a bridge connecting theoretical particle physics with the real world of collider experiments. Yet their computation by means of Feynman diagrams quickly becomes prohibitive, and is only valid at weak coupling. Focusing on the simplest interacting gauge theory, known as large-color maximally supersymmetric Yang - Mills, and exploiting its integrability, in this talk I present a finite-coupling expression for its six-particle amplitude in a particular kinematic limit: The origin in the space of its natural kinematic variables, where two-particle Mandelstam invariants become much smaller than three-particle ones. I also demonstrate that our expression is in perfect agreement with existing field- and string-theoretic predictions for its weak and strong coupling expansion, respectively.

Emergent fields from Hidden sectors

Speaker: Pascal Anastasopoulos
Institution: Vienna University
Time: Tuesday 11 February 2020, 14:15
Venue: 2nd floor seminar room
Abstract: Hidden theories coupled to the SM may provide emergent fields, that are composites/bound-states of the hidden fields. This is motivated by paradigms emerging from the AdS/CFT correspondence but it is a more general phenomenon. We explore the general setup and we focus on axions, graviphotons (or dark photons) and neutrinos.

Consistent truncations of supergravity and twisted 4d Superconformal Field Theories

Speaker: Chris Rosen
Institution: University of Barcelona
Time: Thursday 20 February 2020, 14:15
Venue: 2nd floor seminar room
Abstract: Superconformal field theories (SCFTs) in four dimensions are a cornerstone of contemporary theoretical physics. In the last decade, interesting classes of such theories have been constructed by compactifying six dimensional SCFTs on a Riemann surface. These theories, as well as some of their less supersymmetric deformations, are notable in that they lack a Lagrangian description. A powerful method for exploring the physics of such theories is provided by the methods of gauge/gravity duality. We illustrate this approach by first reviewing how the four dimensional fixed point theories are described by solutions to eleven dimensional supergravity. We then describe new solutions of the 11d theory that holographically encode deformations of the 4d SCFTs. Our techniques allow one to study these deformations in a five dimensional gauged supergravity theory, which arises as a consistent truncation of the 11d theory and greatly simplifies calculations.

Uplifting Runaways and the Tadpole Problem

Speaker: Severin Lust
Institution: Ecole Polytechnique
Time: Tuesday 25 February 2020, 14:15
Venue: 2nd floor seminar room
Abstract: I will discuss a mechanism which can lead to a possible instability of the KKLT construction for de Sitter vacua. The sphere at the tip of a warped deformed conifold throat can be destabilized by antibranes placed in the throat. Consequently, the stabilization of moduli should not be treated independently from the antibrane uplift in KKLT-like scenarios. A similar bound can be found for numerically constructed Klebanov-Strassler black holes. This conifold destabilization mechanism can be avoided by turning on a large amount of flux on the sphere, but tadpole cancelation constraints the hierarchy of scales in a type IIB flux compactification. Even though sufficiently large tadpole bounds can be realized in string theory, they always come at the expense of a large number of moduli. The stabilization of these moduli by fluxes contributes to the tadpole condition as well, reducing the maximal flux on the KS-throat. I will discuss this problem for the example of M-theory on K3 x K3.

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Speaker: Alejandro Cabo-Bizet
Institution: KCL London
Time: Tuesday 03 March 2020, 14:15
Venue: 2nd floor seminar room
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Speaker: Elli Pomoni
Institution: DESY
Time: Thursday 12 March 2020, 14:15
Venue: 2nd floor seminar room
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Speaker: Ioannis Papadimitriou
Institution: KIAS
Time: Thursday 19 March 2020, 14:15
Venue: 2nd floor seminar room
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Speaker: Diego Rodriguez-Gomez
Institution: University of Oviedo
Time: Tuesday 24 March 2020, 14:15
Venue: 2nd floor seminar room
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Speaker: Konstantinos Siampos
Institution: UOA
Time: Tuesday 31 March 2020, 14:15
Venue: 2nd floor seminar room
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Speaker: Konstantinos Siampos
Institution: UOA
Time: Thursday 02 April 2020, 14:15
Venue: 2nd floor seminar room
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Speaker: Aristomenis Donos
Institution: Durham University
Time: Tuesday 07 April 2020, 14:15
Venue: 2nd floor seminar room
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Homogeneous Holographic Viscoelastic Model, Who Are You ?

Speaker: Matteo Baggioli
Institution: IFT, Madrid
Time: Thursday 09 April 2020, 14:15
Venue: 2nd floor seminar room
Abstract: Models with broken translational invariance have attracted a great deal of interest in the holographic community in recent years, especially in relation to their hydrodynamic description and their possible relevance for strange metal phenomenology. Particular emphasis has been given to the so-called homogeneous models, due to their appealing simplicity. Despite the sustained activity in the field, there still remain a number of open questions. In this talk, I will discuss three fundamental points: 1) What is the correct hydrodynamic description for these models ? 2) What are these models describing ? 3) What is the meaning of the universal phase relaxation found in the literature ? I will provide a concrete and definitive resolution to the first point and I will propose a possible physical interpretation which provides simple answers to the rest of the open issues.

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Speaker: Matthew Buican
Institution: QMUL
Time: Thursday 30 April 2020, 14:15
Venue: 2nd floor seminar room
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Speaker: Nicholas Warner
Institution: University of Southern California
Time: Tuesday 05 May 2020, 14:15
Venue: 2nd floor seminar room
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Speaker: Ulf Danielsson
Institution: Uppsala University
Time: Thursday 07 May 2020, 17:15
Venue: 3d floor seminar room (Colloqium)
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